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Microbunch Instability Observations from a THz Detector at Diamond Light Source

DOI: 10.1088/1742-6596/357/1/012037 DOI Help

Authors: W. Shields (John Adams Institute, Royal Holloway, University of London) , R. Bartolini (Diamond Light Source) , G. Boorman (John Adams Institute, Royal Holloway, University of London) , P. Karataev (John Adams Institute, Royal Holloway, University of London) , A. Lyapin (John Adams Institute, Royal Holloway, University of London) , J. Puntree (John Adams Institute, University of Oxford) , G. Rehm (Diamond Light Source)
Co-authored by industrial partner: No

Type: Conference Paper
Conference: IX International Symposium on Radiation from Relativistic Electrons in Periodic Structures
Peer Reviewed: No

State: Published (Approved)
Published: May 2012

Abstract: Diamond Light source is a third generation synchrotron facility dedicated to producing radiation of outstanding brightness, ranging from infra-red to x-rays. The short electron bunches that are accelerated around the storage ring are susceptible to the phenomenon of microbunching instabilities when the bunch charge exceeds a threshold. The primary feature of the microbunch instabilities is the onset of bursts of radiation in the THz range. The high frequencies involved in the emissions make detection and analysis challenging. A 60-90 GHz Schottky Barrier Diode detector was installed to investigate turn by turn evolution of the instabilities.

Journal Keywords: Beam Bunching; Beam Monitoring; Brightness; Electrons; Ghz Range; Instability; Light Sources; Photon Beams; Photon Emission; Radiation Detection; Schottky Barrier Diodes; Semiconductor Detectors; Storage Rings; Synchrotrons; Thz Range; X Radiation

Subject Areas: Physics


Technical Areas: Accelerator Physics

Added On: 04/11/2012 07:39

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